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Sunday, August 14, 2022
Home Gale Crater, home to NASA’s Curiosity Mars rover, shows a new face in this image made using data from the THEMIS camera on NASA’s Mars Odyssey orbiter. The colors come from an image processing method that identifies mineral differences in surface materials and displays them in false colors. (NASA/JPL-Caltech/Arizona State University) Gale Crater, home to NASA's Curiosity Mars rover, shows a new face in this image made using data from the THEMIS camera on NASA's Mars Odyssey orbiter. The colors come from an image processing method that identifies mineral differences in surface materials and displays them in false colors. (NASA/JPL-Caltech/Arizona State University)

Gale Crater, home to NASA’s Curiosity Mars rover, shows a new face in this image made using data from the THEMIS camera on NASA’s Mars Odyssey orbiter. The colors come from an image processing method that identifies mineral differences in surface materials and displays them in false colors. (NASA/JPL-Caltech/Arizona State University)

Gale Crater, home to NASA's Curiosity Mars rover, shows a new face in this image made using data from the THEMIS camera on NASA's Mars Odyssey orbiter. The colors come from an image processing method that identifies mineral differences in surface materials and displays them in false colors. (NASA/JPL-Caltech/Arizona State University)

Gale Crater, home to NASA’s Curiosity Mars rover, shows a new face in this image made using data from the THEMIS camera on NASA’s Mars Odyssey orbiter. The colors come from an image processing method that identifies mineral differences in surface materials and displays them in false colors. (NASA/JPL-Caltech/Arizona State University)

Seen shortly after local Martian sunrise, clouds gather in the summit pit, or caldera, of Pavonis Mons, a giant volcano on Mars, in this image from the Thermal Emission Imaging System (THEMIS) on NASA’s Mars Odyssey orbiter. (NASA/JPL-Caltech/Arizona State University)